Vaata reede, 25 juuli 1997 arhiivi

Päikese aktiivsuse aruanne

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Päikese ja geofüüsikalise aktiivsuse aruanne 1997 Jul 25 2200 UTC
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Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 206 Välja antud 2200Z kuni 25 JUL 1997

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 24-2100Z kuni 25-2100Z

SOLAR ACTIVITY WAS LOW. REGION 8065 (N18W56) HAS CONTINUED TO GROW AND SHOWS THE FORMATION OF SOME MAGNETIC COMPLEXITY, PARTICULARLY IN THE TRAILING PORTION OF THE GROUP WHERE A GAMMA (AND POTENTIALLY A DELTA) CONFIGURATION HAS FORMED. THE INVERSION LINE RUNS IN A MOSTLY EAST-WEST DIRECTION AND IS A GOOD CANDIDATE FOR DEVELOPING SHEAR. THE GROUP PRODUCED NUMEROUS LOW LEVEL C-FLARES TODAY. THE MOST NOTABLE OF THESE WAS A LONG DURATION C4/SN THAT BEGAN AT ABOUT 2015Z, ROSE SLOWLY TO MAXIMUM AT 2035Z, AND WAS DECAYING SLOWLY AT FORECAST ISSUE TIME. THIS EVENT WAS ACCOMPANIED BY STRONG RADIO BURSTS (1600 SFU AT 2695 MHZ), AND TYPE II/IV RADIO SWEEPS. THE TYPE II SHOCK SPEED WAS ESTIMATED TO BE AROUND 900 KM/S. THERE ARE THREE OTHER SPOTTED REGIONS ON THE DISK INCLUDING NEW REGION 8066 (N22E73), BUT THESE REGIONS WERE RELATIVELY CALM COMPARED TO 8065.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE MOSLY LOW. THERE IS A CHANCE FOR AN ISOLATED M-CLASS FLARE FROM REGION 8065 OVER THE NEXT THREE DAYS.
IIA. Summaarne geofüüsikaline aktiivsus 24-2100Z kuni 25-2100Z
THE GEOMAGNETIC FIELD WAS PREDOMINANTLY QUIET. THERE WERE OCCASIONAL UNSETTLED PERIODS, PARTICULARLY AT THE HIGH LATITUDES.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED FOR THE NEXT THREE DAYS. THERE IS A POSSIBILITY FOR ENHANCED ACTIVITY BEGINNING LATE ON THE THIRD DAY IN RESPONSE TO A CORONAL HOLE THAT WILL BE ROTATING INTO A GEOEFFECTIVE POSITION AT THAT TIME.
III. Sündmuste tõenäosus 26 JULkuni 28 JUL
Klass M15%15%15%
Klass X01%01%01%
Prooton01%01%01%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       25 JUL 080
  Prognoositud   26 JUL-28 JUL  082/082/080
  90 päeva keskmine        25 JUL 073
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 24 JUL  015/010
ESTIMATED AFR/AP 25 JUL  005/007
PREDICTED AFR/AP 26 JUL-28 JUL  005/008-005/008-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 26 JUL kuni 28 JUL
A. Keskmistel laiuskraadidel
Aktiivne10%10%20%
Väike torm05%05%10%
Suur-tõsine torm01%01%01%
B. Kõrgetel laiuskraadidel
Aktiivne10%10%25%
Väike torm05%05%15%
Suur-tõsine torm01%01%10%

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